TY - JOUR
T1 - The one-dimensional power spectrum from the SDSS DR14 Lyα forests
AU - Chabanier, Solène
AU - Palanque-Delabrouille, Nathalie
AU - Yèche, Christophe
AU - Goff, Jean Marc Le
AU - Armengaud, Eric
AU - Bautista, Julian
AU - Blomqvist, Michael
AU - Busca, Nicolas
AU - Dawson, Kyle
AU - Etourneau, Thomas
AU - Font-Ribera, Andreu
AU - Lee, Youngbae
AU - Bourboux, Hélion Du Mas Des
AU - Pieri, Matthew
AU - Rich, James
AU - Rossi, Graziano
AU - Schneider, Donald
AU - Slosar, Anže
N1 - Publisher Copyright:
© 2019 IOP Publishing Ltd and Sissa Medialab.
PY - 2019/7/10
Y1 - 2019/7/10
N2 - We present a measurement of the 1D Lyα forest flux power spectrum, using the complete Baryon Oscillation Spectroscopic Survey (BOSS) and first extended-BOSS (eBOSS) quasars at zqso > 2.1, corresponding to the fourteenth data release (DR14) of the Sloan Digital Sky Survey (SDSS). Our results cover thirteen bins in redshift from zLyα = 2.2 to 4.6, and scales up to k = 0.02 (km/s)-1. From a parent sample of 180,413 visually inspected spectra, we selected the 43,751 quasars with the best quality; this data set improves the previous result from the ninth data release (DR9), both in statistical precision (achieving a reduction by a factor of two) and in redshift coverage. We also present a thorough investigation of identified sources of systematic uncertainties that affect the measurement. The resulting 1D power spectrum of this work is in excellent agreement with the one from the BOSS DR9 data.
AB - We present a measurement of the 1D Lyα forest flux power spectrum, using the complete Baryon Oscillation Spectroscopic Survey (BOSS) and first extended-BOSS (eBOSS) quasars at zqso > 2.1, corresponding to the fourteenth data release (DR14) of the Sloan Digital Sky Survey (SDSS). Our results cover thirteen bins in redshift from zLyα = 2.2 to 4.6, and scales up to k = 0.02 (km/s)-1. From a parent sample of 180,413 visually inspected spectra, we selected the 43,751 quasars with the best quality; this data set improves the previous result from the ninth data release (DR9), both in statistical precision (achieving a reduction by a factor of two) and in redshift coverage. We also present a thorough investigation of identified sources of systematic uncertainties that affect the measurement. The resulting 1D power spectrum of this work is in excellent agreement with the one from the BOSS DR9 data.
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U2 - 10.1088/1475-7516/2019/07/017
DO - 10.1088/1475-7516/2019/07/017
M3 - Article
AN - SCOPUS:85072086745
SN - 1475-7516
VL - 2019
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
IS - 7
M1 - 017
ER -